Physics
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007msngr.130...40f&link_type=abstract
The Messenger, vol. 130, p. 40-42
Physics
Scientific paper
The study of gas transport to the inner regions of galaxies is a fundamental aspect in our understanding of the way galaxies evolve. In this context, star-forming nuclear rings are key features as they contain large amounts of gas and are the sites where a significant fraction of the current star formation is taking place in their host galaxies. Here we present some results from a study of how star formation progresses along nuclear star-forming rings in five spiral galaxies, based on near-infrared SINFONI integral-field observations at the VLT.
Böker Torsten
Falcón-Barroso Jesus
Knapen Johan H.
Ryder Stuart
Schinnerer Eva
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